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81.
Seasonal and inter-annual patterns of macroalgal abundance in a Tagus Estuary oyster reef are described. Macroalgal abundance was estimated as canopy percent cover by three permanent point intercept transects over a 7-year period. Four categories were defined, corresponding to bare substrate and three different macroalgal functional-form groups: (1) ULVA, foliose group, included Ulva spp.; (2) GRACIL, terete corticated macrophyte group, included only Gracilaria gracilis; and (3) FILAM, small (<10 cm) filamentous group, including eight species. A canonical correspondence analysis (CCA) showed that: (1) ULVA were associated with long and hot days, being usually dominant during spring and especially summer; (2) FILAM were associated with mild temperatures and relatively long days, abundant in spring but showed frequent peaks in summer; and (3) GRACIL were also favoured by spring season, although associated to lower temperature and less daylight hours than FILAM. GRACIL and FILAM were present throughout the year. On the contrary, ULVA were absent or with low cover during colder periods. A negative correlation between GRACIL and FILAM seems to indicate competition between the two categories. The applied models explained 23.3% of the temporal variance in category abundance. Rainfall negatively affected macroalgal cover, as indicated by the positive correlation between rainfall and bare substrate. Our conclusions are in agreement with previous studies that consider algae as excellent environmental integrators, even on a small scale, due to a strong link between the macroalgal communities and relevant environmental variables. It is also relevant that this study used open-access databases of environmental variables, which open up new possibilities for mining existing data resources in new ways. Due to large inter-annual variability, long-term studies are essential to understand population dynamics in estuarine phytobenthic communities. 相似文献
82.
基于天气雷达风暴识别跟踪信息STI(Storm Tracking Information)拼图技术设计与应用,对该技术在江西雷电、雷暴大风、冰雹等强天气监测预警能力进行了分析。结果显示:通过对江西8部天气雷达的STI产品进行雷达算法解码,建立STI数据库,按照雷达拼图时间间隔,从数据库中调入STI数据进行15 min、30 min、45 min和60 min路径显示,形成多部雷达的组合STI产品。组合STI产品弥补了单部雷达的不足,对于判断未来1 h回波的移动方向、移动速度有明显的指示意义。而密集指向区对应于回波未来位置的确定效果更好,考虑到整体移向的修正位置更佳,在多次飑线、冰雹等强天气过程中得到了验证。组合STI产品还有助于识别回波系统,对于多个系统并存的天气过程中有很好的对照价值。密集指向区的出现说明回波系统进入发展旺盛期,密集指向区的消失预示着回波系统明显减弱。 相似文献
83.
本文分析了2001年2月和3月期间Cluster Ⅱ穿越磁层顶前后的观测资料,检测到13个通量传输事件(FTEs).用多颗卫星磁场测量资料的最小方差分析(MVAB)方法确定FTE的管轴方向(其中6个方向较可靠).FTE管轴方向的分布和低纬处不同,在磁顶法线坐标系LMN中对M轴有较大偏离,比较靠近L轴.deHoffmann Teller(HT)分析指出,13个FTEs都存在一个很好的HT参考系,表明它们以一个准稳的MHD结构运动.对垂直于管轴方向的运动分析表明FTEs并不一定和背景等离子体一起对流,它们可快于或慢于背景流,但FTEs的运动和背景流基本沿相同方向,其间可有一不大的夹角.在HT坐标系中,10个FTEs的等离子体速度接近零, 其他3个FTEs的等离子体速度约为局地Alfven波速的14%,都不符合Walen关系.其中北半球事件的Walen曲线为正斜率,南半球事件为负斜率,这说明等离子体沿磁力线(北半球顺着磁场,南半球逆着磁场)流向磁层. 相似文献
84.
拐卖儿童犯罪屡禁不止,备受社会和学界关注。地理学视角下的已有研究多注重宏观区域定量分析,缺少基于寻亲成功案例聚焦被拐儿童的微观定性分析,尤其对被拐儿童记忆空间与记忆地图的探究不足。文章基于从“宝贝回家”公益平台提取的典型案例,综合运用文本分析、认知地图分析、案例分析等方法,探索寻亲成功的被拐儿童记忆地图模式及其影响因素。结果表明:1)被拐儿童记忆内容由地方性知识、家庭性知识和个体性知识3部分构成。其中,地方性知识包括儿童家乡的自然物理环境与社会文化环境要素;家庭性知识包括儿童原生家庭成员信息、亲缘关系等要素;个体性知识包括儿童自身体貌特征、失踪时穿着等要素。2)被拐儿童记忆空间形成于其日常活动空间,是地理空间与人文情感的结合;随着儿童年龄增长和时代变迁,儿童记忆空间要素产生变化,形成不同阶段不同时代的独特个体记忆,儿童生活环境的变化易塑造混合复杂的记忆空间。3)被拐儿童记忆地图根据其记忆内容及记忆要素类型分为多要素混合式记忆地图(依托多种感官、多要素定位家乡区域)、空间化布局式记忆地图(即手绘完整地图,具有空间性和尺度性)、单要素主导式记忆地图(即以地标和地名为关键要素)3种模式。4)儿童对其日常活动中频繁接触的场所会留下较为深刻印象,家乡环境中独特形状的道路、水域更易使儿童产生记忆,成为寻亲过程中的重要促进因素;地名、方言、习俗组合与地名、地标组合成为寻亲成功的关键要素组合。 相似文献
85.
The major ion composition of Great Artesian Basin groundwater in the lower Namoi River valley is relatively homogeneous in chemical composition. Traditional graphical techniques have been combined with multivariate statistical methods to determine whether subtle differences in the chemical composition of these waters can be delineated. Hierarchical cluster analysis and principal components analysis were successful in delineating minor variations within the groundwaters of the study area that were not visually identified in the graphical techniques applied. Hydrochemical interpretation allowed geochemical processes to be identified in each statistically defined water type and illustrated how these groundwaters differ from one another. Three main geochemical processes were identified in the groundwaters: ion exchange, precipitation, and mixing between waters from different sources. Both statistical methods delineated an anomalous sample suspected of being influenced by magmatic CO2 input. The use of statistical methods to complement traditional graphical techniques for waters appearing homogeneous is emphasized for all investigations of this type. Copyright © 2006 John Wiley & Sons, Ltd. 相似文献
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88.
CHUDongsheng LIANGMeng SHIXin ZHANGLing 《中国海洋大学学报(英文版)》2004,3(1):106-110
1 Introduction Inrecentyearstherehasbeengrowingresearchin terestinthetwo dimensional (2 D )systemtheory .The 2 Dsystemsmayfindapplicationsinareassuchasmarineseismicdataprocessingandimageprocessing .Althoughmoreandmorevaluableresultshavebeengained ,mos… 相似文献
89.
为了解九孔鲍养殖环境中细菌生理菌群的生态作用,对分离自养殖水体的33株菌株的产酶能力和种类进行了研究。结果表明,具有分泌胞外蛋白酶、脂肪酶和纤维素酶能力的菌株分别为39.4%、57.6%和30.3%;在这33株菌中,产至少一种胞外酶的菌株比例高达63.6%。API鉴定结果表明,在有能力分泌胞外蛋白酶、脂肪酶和纤维素酶的菌株中,弧菌菌群所占的比例分别为46%、42%和40%,而其中河流弧菌又占各弧菌菌群比例的83.3%、62.5%和100%。充分阐明弧菌,尤其是河流弧菌为优势菌,在鲍鱼养殖微生物态中起的重要作用。 相似文献
90.
Bo Zhang Yan-Xia Zhang Ji Li Qiu-He Peng Department of Physics Hebei Normal University Shijiazhuang Center of Theoretical Nuclear Physics National Laboratory of Heavy Ion Accelerator Lanzhou National Astronomical Observatories Chinese Academy of Sciences Beijing Department of Astronomy Nanjing University Nanjing 《中国天文和天体物理学报》2002,2(5):429-440
We have collected nearly all the available observed data of the elements from Ba to Dy in halo and disk stars in the metallicity range -4.0 <[Fe/H]< 0.5. Based on the observed data of Ba and Eu, we evaluated the least-squares regressions of [Ba/Fe] on [Fe/H], and [Eu/H] on [Ba/H]. Assuming that the heavy elements (heavier than Ba) are produced by a combination of the main components of s- and r-processes in metal-poor stars, and choosing Ba and Eu as respective representative elements of the main s- and the main r-processes, a statistical model for predicting the Galactic chemical evolution of the heavy elements is presented. With this model, we calculate the mean abundance trends of the heavy elements La, Ce, Pr, Nd, Sm, and Dy with the metallicity. We compare our results with the observed data at various metallicities, showing that the predicted trends are in good agreement with the observed trends, at least for the metallicity range [Fe/H]> -2.5. Finally, we discuss our results and deduce some importa 相似文献